New observations and transit solutions of the exoplanets HAT-P-53b and XO-5b
We present photometric observations of transiting exoplanets HATP-53b and XO-5b by the Rozhen 2 m telescope. The modeling of the HAT-P-53b transit required bigger planet radius than the previously published value due to the bigger depth of the newly-observed transit. The transit solution of...
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Astronomical Observatory, Department of Astronomy, Belgrade
2018-01-01
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doaj-6ab8c183ae8a4ec1a25f1581214624ad2020-11-24T23:18:44ZengAstronomical Observatory, Department of Astronomy, BelgradeSerbian Astronomical Journal1450-698X1820-92892018-01-012018196152010.2298/SAJ1896015K1450-698X1896015KNew observations and transit solutions of the exoplanets HAT-P-53b and XO-5bKjurkchieva Diana0Petrov Nikola1Ibryamov Sunay2Nikolov Grigor3Popov Velimir4Shumen University, Department of Physics, Shumen, BulgariaBulgarian Academy of Sciences, Institute of Astronomy and NAO, Sofia, BulgariaShumen University, Department of Physics, Shumen, BulgariaBulgarian Academy of Sciences, Institute of Astronomy and NAO, Sofia, BulgariaShumen University, Department of Physics, Shumen, BulgariaWe present photometric observations of transiting exoplanets HATP-53b and XO-5b by the Rozhen 2 m telescope. The modeling of the HAT-P-53b transit required bigger planet radius than the previously published value due to the bigger depth of the newly-observed transit. The transit solution of XO-5b led to values of fitted parameters within errors of the previously published results. Based on a time span of around 9 years we improved the orbital period of XO-5b to the value of 4.187751515 d. The quality of our data does not allow determination of planet temperatures by the transit solutions. Our results confirmed the Jupiter type of the two targets. The more bloated nature of HAT-P-53b is a result of its considerable closer orbit and higher temperature of the host star. The best fits of the newly-observed transits of HAT-P-53b and XO-5b correspond to the quadratic limb-darkening law of their host stars whose coefficients were determined. The high sensitivity of the transit solutions to the stellar limb-darkening law and its coefficient( s) is proposed as a tool for precise empirical investigation of the limb-darkening effect of host stars and its interpretation.http://www.doiserbia.nb.rs/img/doi/1450-698X/2018/1450-698X1896015K.pdfStars: planetary systemsTechniques: photometricStars: individual:HAT-P-53, XO-5 |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Kjurkchieva Diana Petrov Nikola Ibryamov Sunay Nikolov Grigor Popov Velimir |
spellingShingle |
Kjurkchieva Diana Petrov Nikola Ibryamov Sunay Nikolov Grigor Popov Velimir New observations and transit solutions of the exoplanets HAT-P-53b and XO-5b Serbian Astronomical Journal Stars: planetary systems Techniques: photometric Stars: individual:HAT-P-53, XO-5 |
author_facet |
Kjurkchieva Diana Petrov Nikola Ibryamov Sunay Nikolov Grigor Popov Velimir |
author_sort |
Kjurkchieva Diana |
title |
New observations and transit solutions of the exoplanets HAT-P-53b and XO-5b |
title_short |
New observations and transit solutions of the exoplanets HAT-P-53b and XO-5b |
title_full |
New observations and transit solutions of the exoplanets HAT-P-53b and XO-5b |
title_fullStr |
New observations and transit solutions of the exoplanets HAT-P-53b and XO-5b |
title_full_unstemmed |
New observations and transit solutions of the exoplanets HAT-P-53b and XO-5b |
title_sort |
new observations and transit solutions of the exoplanets hat-p-53b and xo-5b |
publisher |
Astronomical Observatory, Department of Astronomy, Belgrade |
series |
Serbian Astronomical Journal |
issn |
1450-698X 1820-9289 |
publishDate |
2018-01-01 |
description |
We present photometric observations of transiting exoplanets HATP-53b and
XO-5b by the Rozhen 2 m telescope. The modeling of the HAT-P-53b transit
required bigger planet radius than the previously published value due to the
bigger depth of the newly-observed transit. The transit solution of XO-5b
led to values of fitted parameters within errors of the previously published
results. Based on a time span of around 9 years we improved the orbital
period of XO-5b to the value of 4.187751515 d. The quality of our data does
not allow determination of planet temperatures by the transit solutions. Our
results confirmed the Jupiter type of the two targets. The more bloated
nature of HAT-P-53b is a result of its considerable closer orbit and higher
temperature of the host star. The best fits of the newly-observed transits
of HAT-P-53b and XO-5b correspond to the quadratic limb-darkening law of
their host stars whose coefficients were determined. The high sensitivity of
the transit solutions to the stellar limb-darkening law and its coefficient(
s) is proposed as a tool for precise empirical investigation of the
limb-darkening effect of host stars and its interpretation. |
topic |
Stars: planetary systems Techniques: photometric Stars: individual:HAT-P-53, XO-5 |
url |
http://www.doiserbia.nb.rs/img/doi/1450-698X/2018/1450-698X1896015K.pdf |
work_keys_str_mv |
AT kjurkchievadiana newobservationsandtransitsolutionsoftheexoplanetshatp53bandxo5b AT petrovnikola newobservationsandtransitsolutionsoftheexoplanetshatp53bandxo5b AT ibryamovsunay newobservationsandtransitsolutionsoftheexoplanetshatp53bandxo5b AT nikolovgrigor newobservationsandtransitsolutionsoftheexoplanetshatp53bandxo5b AT popovvelimir newobservationsandtransitsolutionsoftheexoplanetshatp53bandxo5b |
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1725580287586336768 |